Stability of hydrodynamical relativistic planar jets. I. Linear evolution and saturation of Kelvin-Helmholtz modes TeX Export

@misc{citeulike:584192, abstract = {The effects of relativistic dynamics and thermodynamics in the development of Kelvin-Helmholtz instabilities in planar, relativistic jets along the early phases (namely linear and saturation phases) of evolution has been studied by a combination of linear stability analysis and high-resolution numerical simulations for the most unstable first reflection modes in the temporal approach. Three different values of the jet Lorentz factor (5, 10 and 20) and a few different values of specific internal energy of the jet matter (from 0.08 to \$60.0 c^2\$) have been considered. Figures illustrating the evolution of the perturbations are also shown.}, archivePrefix = {arXiv}, author = {Perucho, M. and Hanasz, M. and Marti, J. M. and Sol, H.}, citeulike-article-id = {584192}, citeulike-linkout-0 = {http://arxiv.org/abs/astro-ph/0407548}, citeulike-linkout-1 = {http://arxiv.org/pdf/astro-ph/0407548}, day = {27}, eprint = {astro-ph/0407548}, keywords = {jet, kh, stability}, month = {Jul}, posted-at = {2006-04-12 15:52:28}, priority = {5}, title = {Stability of hydrodynamical relativistic planar jets. I. Linear evolution and saturation of Kelvin-Helmholtz modes}, url = {http://arxiv.org/abs/astro-ph/0407548}, year = {2004} }

TY - ELEC ID - citeulike:584192 L3 - citeulike-article-id:584192 N2 - The effects of relativistic dynamics and thermodynamics in the development of Kelvin-Helmholtz instabilities in planar, relativistic jets along the early phases (namely linear and saturation phases) of evolution has been studied by a combination of linear stability analysis and high-resolution numerical simulations for the most unstable first reflection modes in the temporal approach. Three different values of the jet Lorentz factor (5, 10 and 20) and a few different values of specific internal energy of the jet matter (from 0.08 to $60.0 c^2$) have been considered. Figures illustrating the evolution of the perturbations are also shown. TI - Stability of hydrodynamical relativistic planar jets. I. Linear evolution and saturation of Kelvin-Helmholtz modes KW - jet KW - kh KW - stability AU - Perucho, M AU - Hanasz, M AU - Marti, JM AU - Sol, H PY - 2004/Jul/27/ UR - http://arxiv.org/abs/astro-ph/0407548 ER -